Anisotropic quantum cosmological models: a discrepancy between many-worlds and dBB interpretations
| dc.creator | Alvarenga, F. G. | |
| dc.creator | Batista, A. B. | |
| dc.creator | Fabris, J. C. | |
| dc.creator | Goncalves, S. V. B. | |
| dc.date | 2002-02-04 | |
| dc.date.accessioned | 2026-07-07T03:26:39Z | |
| dc.date.available | 2026-07-07T03:26:39Z | |
| dc.description | In the isotropic quantum cosmological perfect fluid model, the initial singularity can be avoided, while the classical behaviour is recovered asymptotically. We verify if initial anisotropies can also be suppressed in a quantum version of a classical anisotropic model where gravity is coupled to a perfect fluid. Employing a Bianchi I cosmological model, we obtain a "Schrödinger-like" equation where the matter variables play de role of time. This equation has a hyperbolic signature. It can be explicitly solved and a wave packet is constructed. The expectation value of the scale factor, evaluated in the spirit of the many-worlds interpretation, reveals an isotropic Universe. On the other hand, the bohmian trajectories indicate the existence of anisotropies. This is an example where the Bohm-de Broglie and the many-worlds interpretations are not equivalent. It is argued that this inequivalence is due to the hyperbolic structure of the "Schrödinger-like" equation. | |
| dc.description | Latex file, 15 pages, 2 figures | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0202009 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0202009 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/34125 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Quantum Physics | |
| dc.title | Anisotropic quantum cosmological models: a discrepancy between many-worlds and dBB interpretations | |
| dc.type | text |